Results 181 to 190 of about 38,720 (218)

Olfactory dysfunction and all-cause mortality: a systematic review and meta-analysis. [PDF]

open access: yesJ Glob Health
Lin Z   +14 more
europepmc   +1 more source

A "turn-off" photoacoustic contrast for urokinase-type plasminogen activator activity. [PDF]

open access: yesNPJ Biomed Innov
Sharma A   +4 more
europepmc   +1 more source

Tube feet dynamics drive adaptation in sea star locomotion. [PDF]

open access: yesProc Natl Acad Sci U S A
Deridoux A   +5 more
europepmc   +1 more source

The effect of metabolic bariatric surgery on Anti-Müllerian hormone levels: a systematic review and meta-regression analysis. [PDF]

open access: yesBMC Endocr Disord
Mehdinezhad Roshan M   +9 more
europepmc   +1 more source

A Faint Progenitor System for the Faint Supernova 2024vjm

open access: yes
Zimmerman E   +69 more
europepmc   +1 more source

Searching for Low Mass Stars in the Halo

Astrophysics and Space Science, 1999
From microlensing events detected at high galactic latitude as well as from direct measurements of the halo stellar density, estimations of a potential contribution of low mass stars to the mass budget is questioned. Up to now no clear answer has been found for one main reason: the difficulty to observe them in a sufficient volume, which requires deep ...
A.C. Robin, M. Crézé, V. Mohan
openaire   +1 more source

Very Low Mass Stars

Annual Review of Astronomy and Astrophysics, 1987
Very low mass (VLM) stars, which we define here somewhat arbitrarily as those with masses ;$ 0.3 M 0' pose some of the more interesting problems in stellar astrophysics. The physics of their envelopes and atmospheres are more complicated and their structures less well modeled than their more massive counterparts.
James Liebert, Ronald G. Probst
openaire   +2 more sources

Low mass stars

Astrophysics and Space Science, 1994
Low mass stars contribute an important fraction to the mass of our Galaxy. Due to the faintness of these stars a direct investigation of their space distribution and kinematics can be carried out only in the immediate solar neighbourhood. This fact emphasizes the importance of the “Third Catalogue of Nearby Stars” (CNS3) as a probe of the stellar ...
openaire   +1 more source

THE ORIGIN OF LOW MASS STARS

Origins of life and evolution of the biosphere, 1997
Recent evidence indicates that most low mass stars in the Galaxy (< 5 M [symbol: see text]) form alongside massive stars in clusters embedded in giant molecular clouds. Once their parental gas is removed, the fate of these clusters is to disperse and blend into the field population of the galactic disk.
openaire   +2 more sources

Home - About - Disclaimer - Privacy